The Structure of Space-Time Emerging from the Two-Superbody Problem in Chern Simons Supergravity

Details The Structure of Space-Time Emerging from the Two-Superbody Problem in Chern Simons Supergravity The Structure of Space-Time Emerging from the Two-Superbody Problem in Chern Simons Supergravity

1996-09-12

arxiv.org/abs/gr-qc/9609037v1

Phys.Lett. B397 (1997) 81-87

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

10 pages, LaTex

Scientific paper

10.1016/S0370-2693(97)00148-2

We show that the exact solution of the two_superbody problem in N=2 Chern Simons Supergravity in 2+1 dimensions leads to a supermultiplet of space-times. This supersymmetric space-time is characterized by the two gauge invariant observables of the super Poincare' group, which may be viewed as the Casimir invariants of an equivalent one-superbody state. The metric of this space-time supermultiplet can be cast into the form of the metric for a spinning cone in which the coordinates do not commute or for a spinning cone with an additional finite discrete dimension. Some of the interesting features of this universe and their possible physical implications are discussed in the light of a corresponding observation by Witten.

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